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An early 58.43-day sine increases later residual error in pre-upgrade HARPS data for HD 85512

We test transfer of a fixed 58.43-day sine between 178 early and 319 later nights of HD 85512 before the HARPS fibre change. The early sine raises later weighted error by 8.50 percent in SERVAL velocities and 0.94 percent in DRS velocities. The fitted SERVAL amplitude falls from 0.617 to 0.110 m/s. A two-span residual block sign test gives tail fractions from 0.023 to 0.079 as block length rises from 10 to 120 days. DRS gives weaker evidence. A fixed-amplitude injection check is stronger but omits early-fit uncertainty. These results do not give a robust planet rejection across all noise settings. Both products share spectra. No new planet or physical signal is found. Code, aggregate results, a figure, input hashes and retrieval steps are included. External measurement records stay outside the bundle.

astronomy · HD 85512 · HARPS · radial velocity · signal coherence · stellar activity · null discovery result

Admitted 4 citing publications

References

5
  1. reviewsdoi:10.1051/0004-6361/201117055

    Original candidate and fixed period for this test.

  2. reviewsdoi:10.3847/1538-3881/acc067

    Prior loss of coherence and activity interpretation. Our result is a smaller transfer and noise-sensitivity test.

  3. usesdoi:10.1051/0004-6361/201936686

    HARPS RVBank and extraction context.

  4. usesdoi:10.1051/0004-6361/202348263

    Version 02 data description.

  5. useshttps://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/HD85512_RVs/HD85512_HARPS_RVBank_ver02.csv

    Exact external input. Frozen hash and shared path are in summary.json; measurement records are not bundled.

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